{"as_of":"2026-07-16T16:43:00Z","canonical_paper_id":"1009.2209","canonical_url":"https://pith.science/paper/1009.2209/integrity","context_digest":"sha256:22a05da77e4ae8435213e373505458ecaaf17d3f4a544ae2a41304357cc825ad","coverage_summary":[],"findings":[],"findings_empty_copy":"No checks are listed for this paper yet.","findings_observation_state":"no_listed_checks","links":{"arxiv":"https://arxiv.org/abs/1009.2209","bundle_json":"/pith/XFL5KGGIT23NRAEHNAI7SASRAB/bundle.json","citation_record":"/paper/1009.2209/citation-record","evidence":"/evidence","html":"/paper/1009.2209/integrity","integrity_json":"/paper/1009.2209/integrity.json","json":"/paper/1009.2209/integrity.json","legacy_integrity_json":"/pith/1009.2209/integrity.json","paper":"/paper/1009.2209","reference_changes":"/flags?citing=1009.2209"},"paper":{"arxiv_id":"1009.2209","latest_version":1,"primary_cat":"astro-ph.GA","title":"The Prevalence of Narrow Optical Fe II Emission Lines in Type 1 Active Galactic Nuclei"},"pith_number":"pith:2010:XFL5KGGIT23NRAEHNAI7SASRAB","pith_short":"XFL5KGGIT23NRAEHNAI7SASRAB","record":{"arxiv_id":"1009.2209","claim":"As of an unrecorded date, Pith completed 0 of 0 listed checks against arXiv:1009.2209. No listed check completed, so this record makes no findings claim.","counts":{"completed":0,"failed":0,"listed":0,"not_collected":0,"not_requested":0,"partial":0,"public_findings_from_completed":0,"skipped":0,"unavailable":0,"withheld":0},"coverage":[],"observed_at":null,"refusal":"This is a record of named checks, not a clean-status claim or a paper verdict.","schema":"pith.integrity.v1"},"schema":"pith.paper-integrity-record.v1","species":"LEDGER"}